Spectral energy distribution of the emission predicted by our model for LS 5039 for different parts of the orbit and inclinations of the system. Different radiative processes are colour-coded: synchrotron (green lines), inverse Compton (orange), inverse Compton attenuated by γγ-absorption (red), and total (black). The contributions to the total emission from the inner (dashed lines), middle (dashed-dotted), and far regions (dotted) are shown separately (for a description of the regions, see the main text). The model predictions are shown together with observations in soft X-rays (Takahashi et al. 2009) as well as LE (Collmar & Zhang 2014), HE (Hadasch et al. 2012), and VHE (Aharonian et al. 2006) gamma-rays. Results are shown for different parts of the orbit as defined in Fig. 1, with INFC on the top and SUPC on the bottom, and for different inclinations i of the orbital plane, with i = 30° on the left and i = 60° on the right.